Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes

doi:10.3847/1538-4357/ab2f77

	Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes
	Zhang QS(张钱生)1,2,3,4 ; Li Y(李焱)1,2,3,4 ; Christensen-Dalsgaard, Jorgen 5,6
刊名	ASTROPHYSICAL JOURNAL
	2019-08-20
卷号	881 期号:2 页码:26
关键词	convection Sun: abundances Sun: helioseismology Sun: interior
ISSN号	0004-637X
DOI	10.3847/1538-4357/ab2f77
产权排序	第1完成单位
文献子类	Article
英文摘要	Helioseismic observations have revealed many properties of the Sun: the depth and helium abundance of the convection zone, the sound speed, and the density profiles in the solar interior. Those constraints have been used to judge the stellar evolution theory. With the old solar composition (e.g., GS98), the solar standard model is in reasonable agreement with the helioseismic constraints. However, a solar model with a revised composition (e.g., AGSS09) with a low abundance Z of heavy elements cannot be consistent with those constraints. This is the so-called "solar abundance problem," standing for more than 10 yr even with the recent upward revised Ne abundance. Many mechanisms have been proposed to mitigate the problem. However, there is still no low-Z solar model satisfying all helioseismic constraints. In this paper, we report a possible solution to the solar abundance problem. With some extra physical processes that are not included in the standard model, solar models can be significantly improved. Our new solar models with convective overshoot, the solar wind, and early mass accretion show consistency with helioseismic constraints, the solar Li abundance, and observations of solar neutrino fluxes.
学科主题	天文学 ; 恒星与银河系 ; 恒星物理学 ; 恒星形成与演化
URL标识	查看原文
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
资助项目	National Natural Science Foundation of China[11303087] ; National Natural Science Foundation of China[11773064] ; National Natural Science Foundation of China[11333006] ; National Natural Science Foundation of China[11521303] ; foundation of the Chinese Academy of Sciences (Light of West China Program) ; Danish National Research Foundation[DNRF106] ; National Science Foundation[NSF PHY-1748958] ; foundation of the Chinese Academy of Sciences (Youth Innovation Promotion Association)
WOS关键词	LITHIUM DEPLETION ; NUMERICAL SIMULATIONS ; STELLAR CONVECTION ; THERMOHALINE CONVECTION ; CHEMICAL-COMPOSITION ; NONLOCAL CONVECTION ; STARS ; ABUNDANCES ; EVOLUTION ; GRANULATION
WOS研究方向	Astronomy & Astrophysics
语种	英语
出版者	IOP PUBLISHING LTD
WOS记录号	WOS:000482006100002
资助机构	National Natural Science Foundation of China[11303087, 11773064, 11333006, 11521303] ; foundation of the Chinese Academy of Sciences (Light of West China Program) ; Danmarks Grundforskningsfond[DNRF106] ; National Science Foundation (NSF)[NSF PHY-1748958] ; foundation of the Chinese Academy of Sciences (Youth Innovation Promotion Association)
内容类型	期刊论文
源URL	[http://ir.ynao.ac.cn/handle/114a53/20874]
专题	云南天文台_恒星物理研究组云南天文台_中国科学院天体结构与演化重点实验室
通讯作者	Zhang QS(张钱生)
作者单位	1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing 100012, People's Republic of China 3.Key Laboratory for the Structure and Evolution of Celestial Objects, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming 650216, People's Republic of China 4.University of Chinese Academy of Sciences, Beijing 100049, People's Republic of China 5.Stellar Astrophysics Centre and Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark 6.Kavli Institute for Theoretical Physics, University of California, Santa Barbara, CA 93106-4030, USA
推荐引用方式 GB/T 7714	Zhang QS,Li Y,Christensen-Dalsgaard, Jorgen. Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes[J]. ASTROPHYSICAL JOURNAL,2019,881(2):26.
APA	Zhang QS,Li Y,&Christensen-Dalsgaard, Jorgen.(2019).Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes.ASTROPHYSICAL JOURNAL,881(2),26.
MLA	Zhang QS,et al."Solar Models with Convective Overshoot, Solar-wind Mass Loss, and PMS Disk Accretion: Helioseismic Quantities, Li Depletion, and Neutrino Fluxes".ASTROPHYSICAL JOURNAL 881.2(2019):26.